Search results for "methods [Diffusion Tensor Imaging]"

showing 10 items of 992 documents

Asymmetrically Apodized Fiber Bragg Gratings for Applications in Dispersion-Less Fabry-Pérot Fiber Cavities

2010

Abstract This article presents a theoretical study of the dispersion properties of the asymmetrically apodized fiber Bragg gratings. It is shown that the dispersive behavior of these gratings may be changed from normal to anomalous, depending on the apodization function and the grating strength. The asymmetrical Bessel functions were chosen in order to demonstrate these properties of the gratings. The application of this effect in a dispersion-less Fabry-Perot fiber cavity formed by two asymmetrically apodized fiber Bragg gratings is discussed.

PHOSFOSOptical fiberMaterials sciencebusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsLong-period fiber gratingGratingAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materialslaw.inventionOpticsApodizationFiber Bragg gratinglawDispersion (optics)Physics::Atomic PhysicsFiberbusinessFiber and Integrated Optics
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First results on dark matter annihilation in the Sun using the ANTARES neutrino telescope

2013

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was found to be compatible with background expectations. The 90% CL upper limits in terms of spin-dependent and spin-independent WIMP-proton cross-sections are derived and compared to predictions of two sup…

PHOTINOAstrophysicsMASSIVE PARTICLES01 natural sciencesLIMITSDirect searchCANDIDATESPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilationdark matter detectors[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Particle physicsAstrophysics::Instrumentation and Methods for AstrophysicsCAPTURELIGHTparticle physics - cosmology connectionWeakly interacting massive particlesneutrino experiments; particle physics - cosmology connection; dark matter detectors; supersymmetry and cosmologyFísica nuclearNeutrinosupersymmetry andAstrophysics - High Energy Astrophysical PhenomenaCosmology connectionsupersymmetry and cosmologyFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Supersymmetry and cosmologydark matter detectorAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeDark matterFOS: Physical sciencesddc:500.2neutrino experimentsSEARCH0103 physical sciencesDETECTORS010306 general physicsSelection (genetic algorithm)Dark matter detectors010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsNeutrino experimentsFISICA APLICADAParticle physics - cosmology connectionneutrino experimentHigh Energy Physics::ExperimentcosmologySYSTEM
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Comparing equilibration schemes of high-molecular-weight polymer melts with topological indicators.

2021

Abstract Recent theoretical studies have demonstrated that the behaviour of molecular knots is a sensitive indicator of polymer structure. Here, we use knots to verify the ability of two state-of-the-art algorithms—configuration assembly and hierarchical backmapping—to equilibrate high-molecular-weight (MW) polymer melts. Specifically, we consider melts with MWs equivalent to several tens of entanglement lengths and various chain flexibilities, generated with both strategies. We compare their unknotting probability, unknotting length, knot spectra, and knot length distributions. The excellent agreement between the two independent methods with respect to knotting properties provides an addit…

PaperMaterials sciencemolecular knots; multiscale simulations; polymer melts; polymer modelling; topological propertiesStructure (category theory)02 engineering and technologyQuantum entanglementTopologyMultiscale Simulation Methods for Soft Matter Systemspolymer melts01 natural sciencesSpectral lineMolecular dynamicsKnot (unit)multiscale simulationsChain (algebraic topology)Consistency (statistics)0103 physical sciencesGeneral Materials Sciencepolymer modelling010306 general physicsmolecular knotschemistry.chemical_classificationPolymer021001 nanoscience & nanotechnologyCondensed Matter PhysicsMathematics::Geometric Topologychemistry0210 nano-technologytopological properties
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Multi-PeV Signals from a New Astrophysical Neutrino Flux beyond the Glashow Resonance.

2016

The IceCube neutrino discovery was punctuated by three showers with $E_\nu$ ~ 1-2 PeV. Interest is intense in possible fluxes at higher energies, though a marked deficit of $E_\nu$ ~ 6 PeV Glashow resonance events implies a spectrum that is soft and/or cutoff below ~few PeV. However, IceCube recently reported a through-going track event depositing 2.6 $\pm$ 0.3 PeV. A muon depositing so much energy can imply $E_{\nu_\mu} \gtrsim$ 10 PeV. We show that extending the soft $E_\nu^{-2.6}$ spectral fit from TeV-PeV data is unlikely to yield such an event. Alternatively, a tau can deposit this much energy, though requiring $E_{\nu_\tau}$ ~10x higher. We find that either scenario hints at a new flu…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesCosmic ray01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Flux (metallurgy)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physicsGlashow resonanceHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics - Astrophysics of GalaxiesHigh Energy Physics - PhenomenologyAstrophysics of Galaxies (astro-ph.GA)High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)Energy (signal processing)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical review letters
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A test of electric charge conservation with Borexino

2015

Borexino is a liquid scintillation detector located deep underground at the Laboratori Nazionali del Gran Sasso (LNGS, Italy). Thanks to the unmatched radio-purity of the scintillator, and to the well understood detector response at low energy, a new limit on the stability of the electron for decay into a neutrino and a single mono-energetic photon was obtained. This new bound, tau > 6.6 10**28 yr at 90 % C.L., is two orders of magnitude better than the previous limit.

Particle physicsPhysics - Instrumentation and DetectorsOrders of magnitude (temperature)Physics::Instrumentation and DetectorsGeneral Physics and AstronomyFOS: Physical sciencesElectronScintillatorElectric chargeHigh Energy Physics - ExperimentNuclear physicsPhysics and Astronomy (all)High Energy Physics - Experiment (hep-ex)ddc:550Nuclear ExperimentBorexinoComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]Liquid scintillation countingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)High Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Axion search with BabyIAXO in view of IAXO

2020

Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun's core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to backgro…

Particle physicsPhysics - Instrumentation and Detectorssolar axion[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]experimental methodsDark matterFOS: Physical sciences7. Clean energyString (physics)Standard Modelaxion helioscopedesign [detector]International Axion Observatory (IAXO)ObservatoryPeccei-Quinn mechanismDark Matterdetector design[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental TechniquesAxionsun-tracking systemsphysics.ins-detactivity reportdetector: designPhysicsinstrumentationHelioscopeLarge Hadron Colliderdetectorsolar [axion]DESYInstrumentation and Detectors (physics.ins-det)[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]IAXOmagnetopticsaxion: solar
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Search for Dark Matter Annihilations in the Sun with the 79-String IceCube Detector

2012

We have performed a search for muon neutrinos from dark matter annihilation in the center of the Sun with the 79-string configuration of the IceCube neutrino telescope. For the first time, the DeepCore sub-array is included in the analysis, lowering the energy threshold and extending the search to the austral summer. The 317 days of data collected between June 2010 and May 2011 are consistent with the expected background from atmospheric muons and neutrinos. Upper limits are therefore set on the dark matter annihilation rate, with conversions to limits on spin-dependent and spin-independent WIMP-proton cross-sections for WIMP masses in the range 20 - 5000 GeV. These are the most stringent s…

Particle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesGeneral Physics and AstronomyCosmic rayddc:500.2MASSIVE PARTICLESAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)LIMITSWIMP0103 physical sciencesddc:550010306 general physicsLight dark matterCANDIDATESHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsCONSTRAINTSCAPTURENEUTRINOSPhysics and AstronomyNeutrino detector13. Climate actionWeakly interacting massive particlesHigh Energy Physics::ExperimentCryogenic Dark Matter SearchNeutrinoAstrophysics - High Energy Astrophysical PhenomenaPhysical Review Letters
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Minimization of a rectangular patch using genetic algorithms

2002

In recent years, the miniaturization of antennas have become more and more important, especially in connection with subscriber transceivers for cellular systems. Due to the multiple scattering environments and the almost indefinable operating scenario, the crosspolarization characteristics of the antenna are less important, however its physical size is critical. The attempts to reduce the physical size of the antenna made in the past, used classical methods, such as embedding the antenna in a dielectric medium of a high permittivity, adding a resistive element in series with the antenna, etc., but little effort was invested in simply generating other geometries, which by their intrinsic pro…

Patch antennaEngineeringReconfigurable antennaDirectional antennabusiness.industryConformal antennaAntenna measurementAstrophysics::Instrumentation and Methods for AstrophysicsElectrical engineeringEvolved antennaMicrostripAntenna efficiencylaw.inventionMicrostrip antennaElectrical lengthlawElectronic engineeringAntenna (radio)businessOmnidirectional antennaComputer Science::Information TheoryIEEE Antennas and Propagation Society International Symposium. 2001 Digest. Held in conjunction with: USNC/URSI National Radio Science Meeting (Cat. No.01CH37229)
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A FRET-based assay for characterization of alternative splicing events using peptide nucleic acid fluorescence in situ hybridization

2009

We describe a quantitative method for detecting RNA alternative splicing variants that combines in situ hybridization of fluorescently labeled peptide nucleic acid (PNA) probes with confocal microscopy Förster resonance energy transfer (FRET). The use of PNA probes complementary to sequences flanking a given splice junction allows to specifically quantify, within the cell, the RNA isoform generating such splice junction by FRET measure. As a proof of concept we analyzed two alternative splicing events originating from lymphocyte antigen 6 (LY6) complex, locus G5B (LY6G5B) pre-mRNA. These are characterized by the removal of the first intron (Fully Spliced Isoform, FSI) or by retention of suc…

Peptide Nucleic AcidsGene isoformCytoplasmIn situ hybridizationBiologychemistry.chemical_compoundFluorescence Resonance Energy TransferGeneticsmedicineHumansProtein IsoformsspliceRNA MessengerIn Situ Hybridization FluorescenceMicroscopy ConfocalPeptide nucleic acidmedicine.diagnostic_testAlternative splicingIntronPepsin AAlternative SplicingNucleic Acid ProbesFörster resonance energy transferBiochemistrychemistryBiophysicsMethods OnlineCell NucleolusHeLa CellsFluorescence in situ hybridizationNucleic Acids Research
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The Time Calibration System of KM3NeT: The Laser Beacon and the Nanobeacon

2015

The KM3NeT collaboration has started the construction of a deep sea neutrino telescope in the Mediterranean with an instrumented volume of several cubic kilometers. The objective of the KM3NeT telescope is to observe cosmic neutrinos. For this, the detector will consist of a tri-dimensional array of optical modules, each one composed of a pressure resistant glass sphere housing 31 small area photomultipliers. An important element of the KM3NeT detector is the system for the relative time calibration between optical modules with a precision of about 1 ns. The system comprises two independent devices: a nanobeacon inside each optical module for calibration of optical modules in the same verti…

PhotomultiplierComputer sciencebusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsLaserlaw.inventionTelescopeKM3NeTOpticslawCalibrationNeutrinobusiness
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